Titlebook: Mass-Losing Pulsating Stars and their Circumstellar Matter; Observations and The Y. Nakada,M. Honma,M. Seki Book 2003 Springer Science+Busi

機(jī)械

The Galactic Kinematics of Mira Variablesewed. Local Miras in the 145-200day period range show a large asymmetric drift and a high net outward motion in the Galaxy. Interpretations of this phenomenon are considered and (following Feast and Whitelock 2000) it is suggested that they are outlying members of the bulge-bar population and indica

愚蠢人

Harass

craving

發(fā)牢騷

被詛咒的人

The Extended Atmosphere and Evolution of the RV Tauri Star, R Scutistars, but rather commonly seen in Mira variables. The period evolution of this star does not fit with an ordinary post-AGB scenario. Therefore, we argue an alternative choice of the evolutional stage; R Sct is not a post-AGB star but an AGB star in the helium-burning phase of the thermal-pulse cycl

vocation

愛國者

e claim as supermodel Heidi Klum? Many scholars of chemistry do not hesi- te to point out that the names associated with “name reactions” are often not the actual inventors. For instance, the Arndt-Eistert reaction has nothing to do with either Arndt or Eistert, Pummerer did not discover the “Pummer

指耕作

P. R. Wood latest references to these name reactions.Gives representatI don‘t have my name on anything that I don‘t really do. –Heidi Klum Can the organic chemists associated with so-called “Named Reactions” make the same claim as supermodel Heidi Klum? Many scholars of chemistry do not hesi- te to point out

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